This is classified as a C-type asteroid and is probably composed of privitive carbonaceous material. It has very dark surface, with an albedo of 0.040. Photometric measurements made from the Oakley Southern Sky Observatory during 2012 gave a light curve with a period of 7.352 ± 0.003 hours and a variation in brightness of 0.18 ± 0.02 in magnitude. This is consistent with a synodic rotation period of 7.356 ± 0.001 hours determined in 2000.
^Moravec, Patricia; Cochren, Joseph; Gerhardt, Michael et al. (October 2012), Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2012 January-April, Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers39 (4): 213–216, Bibcode:2012MPBu...39..213M.